Extended Data Fig. 7: Contribution of each template component to the γ-ray spectrum averaged over the entire ROI, for our default baseline + Sgr dSph model.
From: Gamma-ray emission from the Sagittarius dwarf spheroidal galaxy due to millisecond pulsars
Components shown are as follows: π0 + brems is the Galactic hadronic plus bremsstrahlung foreground, ICS is the Galactic inverse Compton foreground, 4FGL indicates point sources from the 4th Fermi catalogue, Fermi Bubbles indicates the structured Fermi Bubble template, isotropic is the isotropic γ-ray background, ‘other’ includes the Sun and Moon, Loop I, and the Galactic Centre Excess, and Sgr stream indicates the Sgr dSph. The error bars display 1σ statistical errors.
